Topographic models of the icy Saturn satellites

On its tour through the Saturn system Cassini has acquired hundreds of images of the Saturn satellites with resolutions much improved over the earlier Voyager data. These new images provide multi-spectral information on the surfaces but also multi-stereo coverage that can be used for high-resolution topographic modeling of the satellites. In this talk topographic models of Phoebe, Iapetus, Dione, and Tethys will be presented and implications for formational processes will be discussed